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• W4387044872 startingPage "127" @default.
• W4387044872 abstract "Abstract One of the goals of gravitational-wave astrophysics is to infer the number and properties of the formation channels of binary black holes (BBHs); to do so, one must be able to connect various models with the data. We explore benefits and potential issues with analyses using models informed by population synthesis. We consider five possible formation channels of BBHs, as in Zevin et al. (2021b). First, we confirm with the GWTC-3 catalog what Zevin et al. (2021b) found in the GWTC-2 catalog, i.e., that the data are not consistent with the totality of observed BBHs forming in any single channel. Next, using simulated detections, we show that the uncertainties in the estimation of the branching ratios can shrink by up to a factor of ∼1.7 as the catalog size increases from 50 to 250, within the expected number of BBH detections in LIGO–Virgo–KAGRA's fourth observing run. Finally, we show that this type of analysis is prone to significant biases. By simulating universes where all sources originate from a single channel, we show that the influence of the Bayesian prior can make it challenging to conclude that one channel produces all signals. Furthermore, by simulating universes where all five channels contribute but only a subset of channels are used in the analysis, we show that biases in the branching ratios can be as large as ∼50% with 250 detections. This suggests that caution should be used when interpreting the results of analyses based on strongly modeled astrophysical subpopulations." @default.
• W4387044872 created "2023-09-27" @default.
• W4387044872 creator A5047831308 @default.
• W4387044872 creator A5048613822 @default.
• W4387044872 creator A5085670077 @default.
• W4387044872 date "2023-09-26" @default.
• W4387044872 modified "2023-10-17" @default.
• W4387044872 title "What You Don’t Know Can Hurt You: Use and Abuse of Astrophysical Models in Gravitational-wave Population Analyses" @default.
• W4387044872 cites W1838270195 @default.
• W4387044872 cites W1963527825 @default.
• W4387044872 cites W1965426678 @default.
• W4387044872 cites W1968878579 @default.
• W4387044872 cites W1989170879 @default.
• W4387044872 cites W1994870116 @default.
• W4387044872 cites W2007843551 @default.
• W4387044872 cites W2048695882 @default.
• W4387044872 cites W2054630795 @default.
• W4387044872 cites W2054757488 @default.
• W4387044872 cites W2055151270 @default.
• W4387044872 cites W2069557347 @default.
• W4387044872 cites W2075809310 @default.
• W4387044872 cites W2083453708 @default.
• W4387044872 cites W2087059232 @default.
• W4387044872 cites W2097082581 @default.
• W4387044872 cites W2107110738 @default.
• W4387044872 cites W2115462982 @default.
• W4387044872 cites W2123567195 @default.
• W4387044872 cites W2129760210 @default.
• W4387044872 cites W2157908049 @default.
• W4387044872 cites W2160855100 @default.
• W4387044872 cites W2169311155 @default.
• W4387044872 cites W2207139482 @default.
• W4387044872 cites W2230262155 @default.
• W4387044872 cites W2237829933 @default.
• W4387044872 cites W2254470438 @default.
• W4387044872 cites W2260244587 @default.
• W4387044872 cites W2295393748 @default.
• W4387044872 cites W2482412227 @default.
• W4387044872 cites W2510713096 @default.
• W4387044872 cites W2545747680 @default.
• W4387044872 cites W2575089829 @default.
• W4387044872 cites W2589409690 @default.
• W4387044872 cites W2604642821 @default.
• W4387044872 cites W2611629309 @default.
• W4387044872 cites W2754075545 @default.
• W4387044872 cites W2789083266 @default.
• W4387044872 cites W2807614683 @default.
• W4387044872 cites W2885957034 @default.
• W4387044872 cites W2891084346 @default.
• W4387044872 cites W2891993472 @default.
• W4387044872 cites W2949781771 @default.
• W4387044872 cites W2980421388 @default.
• W4387044872 cites W3098569287 @default.
• W4387044872 cites W3098778082 @default.
• W4387044872 cites W3098821728 @default.
• W4387044872 cites W3099326570 @default.
• W4387044872 cites W3099462218 @default.
• W4387044872 cites W3100139542 @default.
• W4387044872 cites W3100832150 @default.
• W4387044872 cites W3102494827 @default.
• W4387044872 cites W3102842056 @default.
• W4387044872 cites W3103645739 @default.
• W4387044872 cites W3104348061 @default.
• W4387044872 cites W3104917387 @default.
• W4387044872 cites W3105158216 @default.
• W4387044872 cites W3105850678 @default.
• W4387044872 cites W3126705839 @default.
• W4387044872 cites W3128520070 @default.
• W4387044872 cites W3132104923 @default.
• W4387044872 cites W3160629185 @default.
• W4387044872 cites W3162609793 @default.
• W4387044872 cites W3165579283 @default.
• W4387044872 cites W3169294553 @default.
• W4387044872 cites W3172755412 @default.
• W4387044872 cites W3190342835 @default.
• W4387044872 cites W3210546870 @default.
• W4387044872 cites W3212777337 @default.
• W4387044872 cites W3214446395 @default.
• W4387044872 cites W3216670584 @default.
• W4387044872 cites W3216958823 @default.
• W4387044872 cites W3217430213 @default.
• W4387044872 cites W4206487324 @default.
• W4387044872 cites W4211177544 @default.
• W4387044872 cites W4212970780 @default.
• W4387044872 cites W4213226327 @default.
• W4387044872 cites W4224882689 @default.
• W4387044872 cites W4226083230 @default.
• W4387044872 cites W4234856688 @default.
• W4387044872 cites W4283071565 @default.
• W4387044872 cites W4283794171 @default.
• W4387044872 cites W4290772722 @default.
• W4387044872 cites W4296756649 @default.
• W4387044872 cites W4306746299 @default.
• W4387044872 cites W4309648866 @default.
• W4387044872 cites W4311533701 @default.
• W4387044872 cites W4353074908 @default.
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• W4387044872 doi "https://doi.org/10.3847/1538-4357/aced98" @default.

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